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Anisotropic cosmological models of Bianchi types III and V in Lyra's geometry

dc.contributor.authorRam S.; Singh P.
dc.date.accessioned2025-05-24T09:56:10Z
dc.description.abstractExact solutions to Einstein's equations are presented in vacuum and in the presence of stiff matter for spatially homogeneous cosmological models of Bianchi types type III and V in the normal gauge for Lyra's geometry. Solutions represent anisotropic cosmological universes which contract from infinite volume at the initial time singularity T=0 to zero volume as T→∞. Some physical properties of the models are also discussed. © 1992 Plenum Publishing Corporation.
dc.identifier.doihttps://doi.org/10.1007/BF00679969
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/20683
dc.relation.ispartofseriesInternational Journal of Theoretical Physics
dc.titleAnisotropic cosmological models of Bianchi types III and V in Lyra's geometry

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